Jen's Understanding by Design Lesson Plan Template


Copernican Revolution Home

Page history last edited by Jennifer 8 months ago
Established Goals: S:ESS1:11:1.2, S:ESS4:11.3.3

Understanding
  • A valid model can predict the actions of the system it is modeling.
  • All scientific models have limits
  • Scientific theories must be backed up with supporting evidence. I evidence that refutes the theory is found both the evidence and theory must be examined.
  • People tend to ignore evidence that challenges their beliefs and accept evidence the supports them.
Essential Question
  • How does an observer's frame of reference effect their perception?
  • How can the motion of the planets be modeled?
  • What does it take to change accepted scientific thought?
  • Why do people resist paradigm shift in scientific thought
Students will know
  • The motion and action of celestial bodies can best be described by a heliocentric system.
  • Kepler's three Laws can be used to model the motion of any satellite.
Students will be able to
  • Use physical and mathematical models to make predictions about the motion of planets.
  • Collect, analyze, and use data to support or refute a hypothesis.
Performance Task
  • (G) Design and carry out an investigation to identify variables the affect the orbital period of a planet.
  • (R) Science (A) Science Peers (S) The Night Sky (P) Data to support a hypothesis and analysis of this data (S) The student must use the SkyGazer software to collect enough quality data to convince an audience of their peers of their conclusion.

Key Criteria
  • Accuracy and precision of data collection should be within +-5%
  • Students should look at data from at least 5 planets and should include the largest range possible.
  • Students conclusions should be supported by their data

Other Evidence
  • Test on Planetary Motion
  • Mock Trail of Galileo, Kepler, and Copernicus. Students will develop arguments for the Inquisition and defense for the scientist.


Learning Plan
Lesson 1: Kepler's Laws
  1. Watch the 1st 15 minutes of Beyond the Big Bang. (W) (H) Jen has this on DVD. It would be great if someone could convert it to a .mov so we could have greater access to it.
  2. Lecture on Copernicus and Kepler. (E)Motion in Space.pdf
  3. Solve Problems using Kepler's 3 Laws as a class (R) (E)3rd Law.pdf Motion in Space.pdf

Lesson 2: Ellispes
  1. Activity: Modeling planetary motion by drawing elispes (E) (R) (E)Modeling Elliptical Orbits.pdf

Lesson 3: Frame of Reference
  1. Using SkyGazer software students will observe planetary motion from different frames of reference. (H) They will use this data to verify Kepler's Laws. (E) (R) (E)
  2. Using the SkyGazer software students will design and carry out an investigation to identify variables that effect the orbital period of a palnet.(E)

Lesson 4: Mock Trial
  1. Watch the 1st 20 minutes of Galileo's Daughter. (W) (H) The Library has this on DVD. It would be great if someone could convert it to a .mov so we could have greater access to it.
  2. In groups students will develop arguments for the Inquisition against Galileo, Copernicus, or Kepler. They will also put together a defense for Galileo, Copernicus, or Kepler. Three mock trials will be held in class.